The target of the in-situ research of optical activity in extraterrestrial samples stimulated an extended investigation of a GC-MS method based on the derivatization of amino acids by using a mixture of perfluorinated alcohols and perfluorinated anhydrides. Amino acids are converted to their N(O,S)-perfluoroacyl perfluoroalkyl esters in a single-step procedure, using different combinations of the derivatization reagents trifluoroacetic anhydride (TFAA)-2,2,2-trifluoro-1-ethanol (TFE), 2,3,3,4,4,, and heptafluorobutyric anhydride (HFBA)-HFB. The derivatives obtained are analyzed using two different chiral columns: Chirasil-L-Val and g-cyclodextrin (Rt-g-DEXsa) stationary phases which show different and complementary enantiomeric selectivity. The mass spectra of the derivatives are studied, and mass fragmentation patterns are proposed: significant fragment ions can be identified to detect amino acid derivatives. The obtained results are compared in terms of the enantiomeric separation achieved and mass spectrometric response. Linearity studies and the measurement of the limit of detection (LOD) show that the proposed method is suitable for a quantitative determination of enantiomers of several amino acids. The use of the programmed temperature vaporiser (PTV) technique for the injection of the untreated reaction mixture is a promising method for avoiding manual treatment of the sample and decreasing the LOD. KEY WORDS: chirality; amino acids; derivatization; GC-MS; in-situ analysis; planetary explorationThe in-situ search for organic molecules in extraterrestrial environments has been proposed for a better understanding of the solar system origin and the emergence of life on Earth. With this aim, detection of chemical biomarkers, i.e., of organic molecules that play an important role in biochemistry, will be one of the main goals of future space missions. Among the key chemical biomarkers on Earth, 1-3 amino and carboxylic acids which have been synthesized by experimental simulations under plausible prebiotic conditions, 4-6 have been detected in several meteorites 7-13 and in the lunar soil. 14-16 Thus, these chemical species appear to be widespread in the solar system, but they can exist without the presence of life. For this reason, the analysis of their optical activity seems to be a good complementary diagnostic tool to identify the link to a biotic or a prebiotic activity. In fact, almost exclusively L-amino acids are incorporated into proteins during microbial biosynthesis, although various D-amino acids have been found in archaea, yeasts, fungi, plants, insects, mollusks, and other eucaryotic organisms. [17][18][19] Because there are no evident biochemical reasons why L-amino acids should be selected over D-amino acids, it is generally assumed that life elsewhere could be based on either L-or D-amino acids, but not both. [20][21][22] Identifying an excess of D-amino acids in an extraterrestrial sample could provide unambiguous evidence for life that evolves independently from the Earth. [23][24] I...